activity
20062009
most citedDetection of Gamma Rays From a Starburst Galaxy

219 citations · 631 across the 10 of their papers we have counts for

collaborators
Showing 2008Show all

6 papers · 1 filter

astro-ph2008

Sites for Gamma-ray Astronomy in Argentina

A. C. Rovero, G. E. Romero, I. Allekotte +9

We have searched for possible sites in Argentina for the installation of large air Cherenkov telescope arrays and water Cherenkov systems. At present seven candidates are identifie…

astro-ph20088 cited

Implications of the VHE Gamma-Ray Detection of the Quasar 3C279

Markus Boettcher, Anita Reimer, Alan P. Marscher

The MAGIC collaboration recently reported the detection of the quasar 3C279 at > 100 GeV gamma-ray energies. Here we present simultaneous optical (BVRI) and X-ray (RXTE PCA) data f…

astro-ph200834 cited

H.E.S.S. Observations of the Prompt and Afterglow Phases of GRB 060602B

HESS Collaboration, F. Aharonian

We report on the first completely simultaneous observation of a gamma-ray burst (GRB) using an array of Imaging Atmospheric Cherenkov Telescopes which is sensitive to photons in th…

astro-ph200830 cited

Search for Gamma-rays from Dark Matter annihilations around Intermediate Mass Black Holes with the H.E.S.S. experiment

HESS Collaboration, F Aharonian, G. Bertone

The H.E.S.S. array of Cherenkov telescopes has performed, from 2004 to 2007, a survey of the inner Galactic plane at photon energies above 100 GeV. About 400 hours of data have bee…

astro-ph20081 cited

Suzaku observation of TeV blazar the 1ES 1218+304: clues on particle acceleration in an extreme TeV blazar

R. Sato, J. Kataoka, T. Takahashi +3

We observed the TeV blazar 1ES 1218+304 with the X-ray astronomy satellite Suzaku in May 2006. At the beginning of the two-day continuous observation, we detected a large flare in…

astro-ph200865 cited

Discovery of VHE gamma-rays from the high-frequency-peaked BL Lac object RGB J0152+017

HESS Collaboration, F. Aharonian

Aims: The BL Lac object RGB J0152+017 (z=0.080) was predicted to be a very high-energy (VHE; > 100 GeV) gamma-ray source, due to its high X-ray and radio fluxes. Our aim is to unde…